Calibration of the NASA Grc 16″ MASS-flow plugdoi:10.1115/FEDSM2012-72266David DavisDavid J FriedlanderJ David SaundersLancert E Foster
Around a million quasars have been catalogued in the Universe by probing deeper and using new methods for discovery. However, the hardest ones to find seem to be the rarest and brightest specimens. Here we study the properties of the most luminous of all
Mass Outflow from the Nucleus of the Seyfert 1 Galaxy NGC 4151Based on observations made with the NASA/ESA Hubble Space Telescope, obtained from the Data A... Mass Outflow from the Nucleus of the Seyfert 1 Galaxy NGC 4151Based on observations made with the NASA/ESA Hubble Space Telescope,...
(4), Eq. (5) clearly illustrates the limitation of the mass flow rate due to the Hertz-Knudsen equation which shows that the gas pressure in the VDB is not equal to the vapor pressure, but rather reduced by the mass flow leaving the VDB, which in a steady system is the same as ...
The ice-flow model assumes that the depression was excavated due to glacier motion and that there is no calving when the glacier is advancing, as the depression would probably be filled with unlithified sediments (Nick et al., 2007). Consequently, the calving module was activated during the ...
Across the Antarctic ice sheet, the temperature at the ice-bed interface – basal temperature – is critical in maintaining the ice sheet’s configuration through its influence on basal sliding, subglacial hydrology, and ice-flow regime1,2,3,4. While frozen bed conditions beneath the continental...
The rate of change of the inertia tensor is estimated by the following equation. ˙I=Ifull−Iemptymfull−mempty˙m The integration of the rate of change of the quaternion vector is given below. ⎡⎢⎢⎢⎢⎢⎣˙q0˙q1˙q2˙q3⎤⎥⎥⎥⎥⎥⎦=−1/2⎡⎢⎢...
Axisymmetric Inlet Flow at Low Supersonic Mach Numbers A calculation method for transonic flow around axisymmetric inlets in subsonic free streams has been extended to work in supersonic free streams. The full potential equation is solved in non-conservative and almost conservative (quasi-co... BG...
This assumption leads to slightly larger contributions from short-range correlations than with further propagation to the second propagation step between discontinuous glaciers (equation (6)). Uncertainties are largely dominated by short- to long-range spatial correlations. d, Comparison of specific-...
This equation assumes that the potential energy is completely converted to kinetic energy. Turnbull (2011) provides an equation that describes the specific energy required for local melting to occur during a mass movement event, Em, and is given by Em=Cp(Tf−Ta)+ζwhere Cp is the specific ...